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XMM Newton

XMM-Newton
XMM-Newton spacecraft model.png
Artist's impression of the XMM-Newton spacecraft
Names High Throughput X-ray Spectroscopy Mission
X-ray Multi-Mirror Mission
Mission type X-ray astronomy
Operator European Space Agency
COSPAR ID 1999-066A
SATCAT no. 25989
Website http://sci.esa.int/xmm-newton/
http://xmm.esac.esa.int/
Mission duration Planned: 2 years
Elapsed: 17 years, 9 months and 5 days
Spacecraft properties
Manufacturer Dornier Satellitensysteme, Carl Zeiss, Media Lario, Matra Marconi Space, BPD Difesa e Spazio, Fokker Space
Launch mass 3,764 kg (8,298 lb)
Dry mass 3,234 kg (7,130 lb)
Dimensions Length: 10.8 m (35 ft)
Span: 16.16 m (53 ft)
Power 1,600 watts
Start of mission
Launch date 10 December 1999, 14:32 (1999-12-10UTC14:32) UTC
Rocket Ariane 5G No. 504
Launch site Guiana Space Centre ELA-3
Contractor Arianespace
Entered service 1 July 2000
Orbital parameters
Reference system Geocentric
Semi-major axis 65,648.3 km (40,792.0 mi)
Eccentricity 0.816585
Perigee 5,662.7 km (3,518.6 mi)
Apogee 112,877.6 km (70,138.9 mi)
Inclination 67.1338 degrees
Period 2789.9 minutes
Epoch 4 February 2016, 01:06:30 UTC
Main telescope
Type 3 × Wolter type-1
Diameter Outer mirror: 70 cm (28 in)
Inner mirror: 30.6 cm (12 in)
Focal length 7.5 m (25 ft)
Collecting area 4,425 cm2 (686 sq in) at 1.5 keV
1,740 cm2 (270 sq in) at 8 keV
Wavelengths 0.1–12 nm (0.1–12 keV)
Resolution 5 to 14 arcseconds

XMM-Newton mission insignia
ESA astrophysics insignia for XMM-Newton

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XMM-Newton mission insignia
ESA astrophysics insignia for XMM-Newton

XMM-Newton, also known as the High Throughput X-ray Spectroscopy Mission and the X-ray Multi-Mirror Mission, is an X-ray space observatory launched by the European Space Agency in December 1999 on an Ariane 5 rocket. It is the second cornerstone mission of ESA's Horizon 2000 programme. Named after physicist and astronomer Sir Isaac Newton, the spacecraft is tasked with investigating interstellar X-ray sources, performing narrow- and broad-range spectroscopy, and performing the first simultaneous imaging of objects in both X-ray and optical (visible and ultraviolet) wavelengths.

Originally scheduled for a two-year mission, the spacecraft remains in good health and has received mission extensions through 2016. ESA plans to succeed XMM-Newton with the Advanced Telescope for High Energy Astrophysics (ATHENA), the second large mission in the Cosmic Vision 2015-25 plan, to be launched in 2028. Its mission is similarly to NASA's Chandra X-ray Observatory, also launched in 1999.

As of May 2017, more than 5,000 papers have been published about either XMM-Newton or the scientific results it has returned.

The observational scope of XMM-Newton includes the detection of X-ray emissions from astronomical objects, detailed studies of star-forming regions, investigation of the formation and evolution of galaxy clusters, the environment of supermassive black holes and mapping of the mysterious dark matter.


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